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Mass of Newtonian stars in the relativistic theory of gravitation and in general relativity
A. A. Vlasov
Abstract:
Unlike RTG, mass of a Newtonian star cannot be determined uniquely from the
equations of GRT and depends on arbitrary choice of coordinate conditions.
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Theoretical and Mathematical Physics, 1987, 73:1, 1124–1129
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Received: 29.05.1986
Citation:
A. A. Vlasov, “Mass of Newtonian stars in the relativistic theory of gravitation and in general relativity”, TMF, 73:1 (1987), 154–160; Theoret. and Math. Phys., 73:1 (1987), 1124–1129
Citation in format AMSBIB
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\paper Mass of Newtonian stars in the relativistic theory of gravitation and in general relativity
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\yr 1987
\vol 73
\issue 1
\pages 154--160
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\transl
\jour Theoret. and Math. Phys.
\yr 1987
\vol 73
\issue 1
\pages 1124--1129
\crossref{https://doi.org/10.1007/BF01022972}
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http://mi.mathnet.ru/eng/tmf5615 http://mi.mathnet.ru/eng/tmf/v73/i1/p154
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